Primordial non-Gaussianity from the large-scale structure
By V. Desjacques, Uros Seljak. 2010
149 citations recorded by the source corpus.
Primordial non-Gaussianity is a potentially powerful discriminant of the physical mechanisms that generate the cosmological fluctuations observed today. Any detection of non-Gaussianity would have profound implications for our understanding of cosmic structure formation. In this paper, we review past and current efforts in the search for primordial non-Gaussianity in the large-scale structure of the Universe.
Subfields: Astronomy and Astrophysics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/bfd26d987e8b722ab94a960bf6065c21975cb41f
How researchers see this paper
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In Astronomy and Astrophysics
- Daniel J. Eisenstein
- Uros Seljak
- F. Beutler
- C. Porciani
- A. Pillepich
- Tommaso Giannantonio
- Adam Amara
- J. Carron
In Statistical and Nonlinear Physics
- Uros Seljak
- Daniel J. Eisenstein
- F. Beutler
- Yu Feng
- Zachary Slepian
- Adam Amara
- Yin Li
- Tommaso Giannantonio
Citations in the corpus
- nbodykit: An Open-source, Massively Parallel Toolkit for Large-scale Structure (2017, background): “…other important questions in contemporary cosmology, including deviations from General Relativity (Mueller et al. 2016), the neutrino mass scale (Lesgourgues & Pastor 2006; Beutler et al. 2014), and the existence of primordial non-Gaussianity (Slosar et al. 2008; Desjacques & Seljak 2010).”
- Computing the Three-Point Correlation Function of Galaxies in $\mathcal{O}(N^2)$ Time (2015, background): “Generically, inflation must couple to ordinary matter so as to produce it during reheating, and this coupling produces some level of non-Gaussianity (Desjacques & Seljak 2010, for a recent review).”
- Constraining primordial non-Gaussianity with future galaxy surveys (2011, methodology): “…deviations) are required to reproduce the N-body results when dark-matter haloes in the simulations are identified using either the friends-of-friends (FoF) or the spherical overdensity (SO) method: this makes unclear which value should be actually used for galaxies (Desjacques & Seljak 2010).”
- Particle production during inflation and gravitational waves detectable by ground-based interferometers (2011, background): “1 Mpc − 1 (see [37] for a recent review), which correspond to scales that left the horizon about N C − 5 efoldings before the end of inflation.”